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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2693
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dc.contributor.authorSivaram, C-
dc.contributor.authorde Sabbata, Venzo-
dc.date.accessioned2008-07-16T05:31:00Z-
dc.date.available2008-07-16T05:31:00Z-
dc.date.issued1991-02-
dc.identifier.citationAstrophysics and Space Science , Vol. 176, No. 1, pp. 145 - 148en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/2693-
dc.description.abstractThe maximum acceleration at the Planck epoch is shown to be related to the maximum magnetic field and curvature as well as temperature in that era. Spin-torsion effects at that epoch also lead to same value.en
dc.format.extent277105 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1991Ap%26SS.176..145Sen
dc.relation.urihttp://www.springerlink.com/content/n87m71k7r0151106/?p=ebf6c406af654d2a884986fde28dd489&pi=13en
dc.subjectAcceleration (Physics)en
dc.subjectBig bang cosmologyen
dc.subjectMagnetic fluxen
dc.subjectParticle accelerationen
dc.subjectParticle accelerationen
dc.subjectSpace-time functionsen
dc.subjectAstronomical modelsen
dc.subjectGravitational effectsen
dc.subjectMagnetic fieldsen
dc.subjectRelativistic effectsen
dc.subjectTorsionen
dc.titleMaximum acceleration and magnetic field in the early universeen
dc.typeArticleen
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